Quantum ESPRESSO Input¶
The input to the QuantumESPRESSO engine has a similar structure as the input to the pw.x executable, with some exceptions.
Note
In the input file there are two System blocks:
The AMS driver System block contains the atomic species, atomic positions, atomic masses (isotopes), and lattice vectors, just like for any other AMS calculation. On each atom line you can also specify for example
QE.label=Fe1
(max 3 characters) to set the internal QE atom type for that atom. See the Examples.The QuantumESPRESSO Engine System block contains keywords from the
&SYSTEM
namelist in the pw.x input file. For example,ecutwfc
to set the plane-wave energy cutoff, as well as many other input options for magnetization, occupations, dispersion corrections, etc. This block is described in detail below.
Pseudopotentials¶
A library of pseudopotentials is included with the AMS Quantum ESPRESSO package. Simply specify the family and the functional in the input and the corresponding pseudopotential files will be used.
The pseudopotentials will also determine the exchange-correlation functional used, unless you set manually set the DFT functional (input_dft) option.
Important
Use an energy cutoff that is large enough for your selected pseudopotentials!
Pseudopotentials
Directory string
Family [Dojo | GBRV | pslibrary-PAW | pslibrary-US | SG15 | SSSP-Efficiency | SSSP-Precision]
Files
Label string
Path string
End
FullyRelativistic Yes/No
Functional [BLYP | LDA | PBE | PBEsol | PW91]
End
Pseudopotentials
- Type:
Block
- Description:
Selects the pseudopotential to use for the atomic species.
Directory
- Type:
String
- Description:
This key is mutually exclusive with the
Family
andFiles
keywords. This key specifies a directory containing label.upf files. Example: System Atoms H 0 0 0 H 0 0 1 QE.Label=H1 H 0 0 2 QE.Label=H2 C 0 0 3 QE.Label=C1 End End This will look for the files H.upf, H1.upf, H2.upf, C1.upf. If H1.upf does not exist, H.upf will be used. If H2.upf does not exist, H.upf will be used. If C1.upf does not exist, C.upf will be used.
Family
- Type:
Multiple Choice
- Default value:
SSSP-Efficiency
- Options:
[Dojo, GBRV, pslibrary-PAW, pslibrary-US, SG15, SSSP-Efficiency, SSSP-Precision]
- GUI name:
Pseudopotential family
- Description:
The pseudopotential family to use. Mutually exclusive with the
Files
andDirectory
keywords.
Files
- Type:
Block
- Recurring:
True
- Description:
Selects the pseudopotentials to use for each atomic species. This key is mutually exclusive with the
Family
andDirectory
keywords.
Label
- Type:
String
- Description:
Label for an atom corresponding to the QE.Label, or to the element symbol if QE.Label is not set.
Path
- Type:
String
- Description:
Path to a .upf file to use as pseudopotential. Relative paths are relative to root of the pseudopotential library shipped with AMS. Prefix a path with ‘./’ to make it relative to the starting directory of your job.
FullyRelativistic
- Type:
Bool
- Default value:
No
- GUI name:
Pseudopotential fully relativistic
- Description:
Whether to use fully relativistic pseudopotentials (required for spin-orbit calculations).
Functional
- Type:
Multiple Choice
- Default value:
PBE
- Options:
[BLYP, LDA, PBE, PBEsol, PW91]
- GUI name:
Pseudopotential functional
- Description:
Exchange-correlation functional that was used to generate the pseudopotential. Not all choices are valid for all pseudopotential families. This functional will also be used for the calculation, unless the
input_dft
option is set.
K-space and k-point sampling¶
The K_Points block corresponds to the K_POINTS card in the pw.x input.
Gamma-point (Γ-point) sampling (fast implementation, not compatible with all calculation types or postprocessing programs):
Engine QuantumEspresso
K_Points gamma
End
EndEngine
Gamma-point (Γ-point) sampling (slower implementation):
Engine QuantumEspresso
K_Points automatic
1 1 1 0 0 0
End
EndEngine
Monkhorst-Pack 6 x 6 x 4 grid, shifted:
Engine QuantumEspresso
K_Points automatic
6 6 4 1 1 1
End
EndEngine
Monkhorst-Pack 6 x 6 x 4 grid, unshifted:
Engine QuantumEspresso
K_Points automatic
6 6 4 0 0 0
End
EndEngine
The output contains details about the generated k-point grid. For further information, see the pw.x documentation.
For DOS and band structure calculations, the main K_Points
block
specifies the k-points used during the self-consistent-field (SCF). The DOS and band structure sections for how to
specify a different k-space sampling for the non-self-consistent parts of DOS
and band structure calculations.
K_Points
- Type:
Non-standard block
- Description:
Specify the k-points to use. Available header values are:
tpiba
,automatic
,crystal
,gamma
,tpiba_b
,crystal_b
,tpiba_c
,crystal_c
, andams_kpath
. See the examples and QE documentation for details. If omitted, onlygamma
is used. For most cases,automatic
(which generates a Monkhorst-Pack grid) is recommended. Note: Gamma-point calculations are significantly faster usinggamma
thanautomatic
, but may not be possible to use for all types of calculations or postprocessing programs.
Control block: dipole/electric field¶
See also
Control
dipfield Yes/No
lelfield Yes/No
tefield Yes/No
End
Control
- Type:
Block
- Description:
Keywords from the &CONTROL namelist in the QuantumEspresso input file.
dipfield
- Type:
Bool
- Default value:
No
- GUI name:
Dipole field
- Description:
If True (and
tefield
is True) a dipole correction is also added to the bare ionic potential - implements the recipe of L. Bengtsson, PRB 59, 12301 (1999). See keywordsedir
,emaxpos
,eopreg
for the form of the correction. Must be used ONLY in a slab geometry, for surface calculations, with the discontinuity FALLING IN THE EMPTY SPACE.
lelfield
- Type:
Bool
- Default value:
No
- GUI name:
Homogeneous E-field
- Description:
If True a homogeneous finite electric field described through the modern theory of the polarization is applied. This is different from setting
tefield
to True!
tefield
- Type:
Bool
- Default value:
No
- GUI name:
Saw-like E-field
- Description:
If True a saw-like potential simulating an electric field is added to the bare ionic potential. See keywords
edir
,eamp
,emaxpos
,eopreg
for the form and size of the added potential.
Electrons block: SCF convergence¶
Electrons
conv_thr float
diagonalization [Davidson | ConjugateGradient | PPCG | ParO | RMM-Davidson | RMM-ParO]
electron_maxstep integer
mixing_beta float
mixing_mode [Plain | Thomas-Fermi | Local-Thomas-Fermi]
mixing_ndim integer
End
Electrons
- Type:
Block
- Description:
Keywords from the &ELECTRONS namelist in the QuantumEspresso input file.
conv_thr
- Type:
Float
- Default value:
1e-06
- Unit:
Rydberg
- GUI name:
Convergence threshold
- Description:
Convergence threshold for selfconsistency: estimated energy error <
conv_thr
. Note thatconv_thr
is extensive, like the total energy.
diagonalization
- Type:
Multiple Choice
- Default value:
Davidson
- Options:
[Davidson, ConjugateGradient, PPCG, ParO, RMM-Davidson, RMM-ParO]
- GUI name:
Diagonalization
- Description:
Available options are: • Davidson: iterative diagonalization with overlap matrix. Fast, may in some rare cases fail. • ConjugateGradient: Conjugate-gradient-like band-by-band diagonalization. MUCH slower than
Davidson
but uses less memory and is (a little bit) more robust. • PPCG: PPCG iterative diagonalization • ParO: ParO iterative diagonalization • RMM-Davidson & RMM-ParO: RMM-DIIS iterative diagonalization. To stabilize the SCF loop RMM-DIIS is alternated with calls to Davidson or ParO solvers.
electron_maxstep
- Type:
Integer
- Default value:
100
- GUI name:
Maximum # SCF iterations
- Description:
Maximum number of iterations in a SCF step.
mixing_beta
- Type:
Float
- Default value:
0.3
- GUI name:
Beta
- Description:
Mixing factor for self-consistency. Note: the default value in the AMS interface (0.3) is smaller than the default value in pw.x (0.7)
mixing_mode
- Type:
Multiple Choice
- Default value:
Plain
- Options:
[Plain, Thomas-Fermi, Local-Thomas-Fermi]
- GUI name:
Mixing mode
- Description:
Available options are: • Plain: charge density Broyden mixing • Thomas-Fermi: as above, with simple Thomas-Fermi screening (for highly homogeneous systems) • Local-Thomas-Fermi: as above, with local-density-dependent TF screening (for highly inhomogeneous systems)
mixing_ndim
- Type:
Integer
- Default value:
8
- GUI name:
Dimension
- Description:
Number of iterations used in mixing scheme. If you are tight with memory, you may reduce it to 4 or so.
System block (in the QuantumESPRESSO engine)¶
Overview:
System
assume_isolated [Auto | None | Martyna-Tuckerman | ESM | 2D]
degauss float
dftd3_threebody Yes/No
dftd3_version [2 | 3 | 4 | 5 | 6]
eamp float
ecutfock float
ecutrho float
ecutvcut float
ecutwfc float
edir [1 | 2 | 3]
emaxpos float
eopreg float
exx_fraction float
exxdiv_treatment [gygi-baldereschi | vcut_spherical | vcut_ws | none]
input_dft string
lspinorb Yes/No
nbnd integer
nqx1 integer
nqx2 integer
nqx3 integer
nr1 integer
nr1s integer
nr2 integer
nr2s integer
nr3 integer
nr3s integer
nspin [None | Collinear | Non-Collinear]
occupations [Smearing | Tetrahedra | Tetrahedra_lin | Tetrahedra_opt | Fixed]
screening_parameter float
smearing [Gaussian | Methfessel-Paxton | Marzari-Vanderbilt | Fermi-Dirac]
starting_magnetization
Label string
Value float
End
tot_magnetization float
vdw_corr [None | Grimme-D2 | Grimme-D3 | TS | MBD | XDM]
x_gamma_extrapolation Yes/No
xdm_a1 float
xdm_a2 float
End
Cutoffs¶
System
ecutrho float
ecutwfc float
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
ecutrho
- Type:
Float
- Unit:
Rydberg
- GUI name:
Charge density cutoff
- Description:
Kinetic energy cutoff for charge density and potential. If this key is not specified and the
Pseudopotential%Family
recommends a ratio ofecutrho
toecutwfc
, this recommended ratio will be used. If there is no recommended ratio, the default value is4 x ecutwfc
. For norm-conserving pseudopotential you should stick to the default value, you can reduce it by a little but it will introduce noise especially on forces and stress. If there are ultrasoft PP, a larger value than the default is often desirable (ecutrho
= 8 to 12 timesecutwfc
, typically). PAW datasets can often be used at4 x ecutwfc
, but it depends on the shape of augmentation charge: testing is mandatory. The use of gradient-corrected functional, especially in cells with vacuum, or for pseudopotential without non-linear core correction, usually requires an higher values ofecutrho
to be accurately converged.
ecutwfc
- Type:
Float
- Default value:
40.0
- Unit:
Rydberg
- GUI name:
Wavefunction energy cutoff
- Description:
Kinetic energy cutoff for wavefunctions.
See also
Number of bands (nbnd)¶
System
nbnd integer
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
nbnd
- Type:
Integer
- GUI name:
Number of bands
- Description:
Number of electronic states (bands) to be calculated. Note that in spin-polarized calculations the number of k-point, not the number of bands per k-point, is doubled. Default: For an insulator, nbnd = number of valence bands (nbnd = # of electrons /2); for a metal, 20% more (minimum 4 more)
Fractional occupation, smearing¶
System
degauss float
occupations [Smearing | Tetrahedra | Tetrahedra_lin | Tetrahedra_opt | Fixed]
smearing [Gaussian | Methfessel-Paxton | Marzari-Vanderbilt | Fermi-Dirac]
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
degauss
- Type:
Float
- Default value:
0.0
- Unit:
Rydberg
- GUI name:
Smearing width
- Description:
Value of the gaussian spreading for Brillouin-zone integration in metals.
occupations
- Type:
Multiple Choice
- Default value:
Fixed
- Options:
[Smearing, Tetrahedra, Tetrahedra_lin, Tetrahedra_opt, Fixed]
- GUI name:
Occupations
- Description:
Available options are: • Smearing: gaussian smearing for metals; see keywords
smearing
anddegauss
• Tetrahedra: Tetrahedron method, Bloechl’s version: P.E. Bloechl, PRB 49, 16223 (1994). Requires uniform grid of k-points, to be automatically generated (seeblock K_Points
). Well suited for calculation of DOS, less so (because not variational) for force/optimization/dynamics calculations. • Tetrahedra_lin: Original linear tetrahedron method. To be used only as a reference; the optimized tetrahedron method is more efficient. • Tetrahedra_opt: optimized tetrahedron method, see M. Kawamura, PRB 89, 094515 (2014). Can be used for phonon calculations as well. • Fixed: for insulators with a gap.
smearing
- Type:
Multiple Choice
- Default value:
Gaussian
- Options:
[Gaussian, Methfessel-Paxton, Marzari-Vanderbilt, Fermi-Dirac]
- GUI name:
Smearing
- Description:
Available options are: • Gaussian: ordinary Gaussian spreading • Methfessel-Paxton: first-order spreading (see PRB 40, 3616 (1989)) • Marzari-Vanderbilt: cold smearing (see PRL 82, 3296 (1999)) • Fermi-Dirac: smearing with Fermi-Dirac function
Magnetization, spin, spin-orbit¶
System
lspinorb Yes/No
nspin [None | Collinear | Non-Collinear]
starting_magnetization
Label string
Value float
End
tot_magnetization float
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
lspinorb
- Type:
Bool
- GUI name:
Spin-orbit
- Description:
if .TRUE. the noncollinear code can use a pseudopotential with spin-orbit.
nspin
- Type:
Multiple Choice
- Default value:
None
- Options:
[None, Collinear, Non-Collinear]
- GUI name:
Magnetization
- Description:
Available options are: • None: not spin-polarized • Collinear: LSDA with magnetization along z-axis • Non-Collinear: any magnetization (equivalent to setting the
noncolin
key to True)
starting_magnetization
- Type:
Block
- Recurring:
True
- Description:
Starting spin polarization for an atomic type in a spin polarized (LSDA or noncollinear/spin-orbit) calculation. Allowed values range between -1 (all spins down for the valence electrons of atom type ‘i’) to 1 (all spins up). If you expect a nonzero magnetization in your ground state, you MUST either specify a nonzero value for at least one atomic type, or constrain the magnetization using keyword
tot_magnetization
for LSDA,constrained_magnetization
for noncollinear/spin-orbit calculations. If you don’t, you will get a nonmagnetic (zero magnetization) state. In order to perform LSDA calculations for an antiferromagnetic state, define two different atomic species corresponding to sublattices of the same atomic type. Note: If you fix the magnetization withtot_magnetization
, do not specifystarting_magnetization
. Note: In the noncollinear/spin-orbit case, starting with zero starting_magnetization on all atoms imposes time reversal symmetry. The magnetization is never calculated and is set to zero.
Label
- Type:
String
- Description:
Label for an atom corresponding to the QE.Label, or to the element symbol if QE.Label is not set.
Value
- Type:
Float
- Description:
Starting magnetization value.
tot_magnetization
- Type:
Float
- GUI name:
Fix total magnetization
- Description:
Total majority spin charge minus minority spin charge. Used to impose a specific total electronic magnetization. If unspecified then tot_magnetization variable is ignored and the amount of electronic magnetization is determined during the self-consistent cycle.
Dispersion corrections¶
Tip
You can access Grimme’s D4 dispersion through an AMS engine addon.
System
vdw_corr [None | Grimme-D2 | Grimme-D3 | TS | MBD | XDM]
dftd3_version [2 | 3 | 4 | 5 | 6]
dftd3_threebody Yes/No
xdm_a1 float
xdm_a2 float
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
vdw_corr
- Type:
Multiple Choice
- Default value:
None
- Options:
[None, Grimme-D2, Grimme-D3, TS, MBD, XDM]
- GUI name:
Dispersion correction
- Description:
Type of Van der Waals correction. Allowed values: • Grimme-D2: Semiempirical Grimme’s DFT-D2, see S. Grimme, J. Comp. Chem. 27, 1787 (2006) [doi:10.1002/jcc.20495], and V. Barone et al., J. Comp. Chem. 30, 934 (2009) [doi:10.1002/jcc.21112]. • Grimme-D3: Semiempirical Grimme’s DFT-D3, see S. Grimme et al, J. Chem. Phys 132, 154104 (2010) [doi:10.1063/1.3382344]. • TS: Tkatchenko-Scheffler dispersion corrections with first-principle derived C6 coefficients, see A. Tkatchenko and M. Scheffler, PRL 102, 073005 (2009). • MBD: Many-body dispersion (MBD) correction to long-range interactions, see A. Ambrosetti, A. M. Reilly, R. A. DiStasio, A. Tkatchenko, J. Chem. Phys. 140 18A508 (2014). • XDM: Exchange-hole dipole-moment model, see A. D. Becke et al., J. Chem. Phys. 127, 154108 (2007) [doi:10.1063/1.2795701], and A. Otero de la Roza et al., J. Chem. Phys. 136, 174109 (2012) [doi:10.1063/1.4705760]. Note that non-local functionals (eg vdw-DF) are NOT specified here but using the
input_dft
keyword.
dftd3_version
- Type:
Multiple Choice
- Default value:
3
- Options:
[2, 3, 4, 5, 6]
- GUI name:
Version
- Description:
Version of Grimme implementation of Grimme-D3: • 2: Original Grimme-D2 parametrization • 3: Grimme-D3 (zero damping) • 4: Grimme-D3 (BJ damping) • 5: Grimme-D3M (zero damping) • 6: Grimme-D3M (BJ damping) • NOTE: not all functionals are parametrized.
dftd3_threebody
- Type:
Bool
- Default value:
Yes
- GUI name:
Use three-body terms
- Description:
Turn three-body terms in Grimme-D3 on. If False two-body contributions only are computed, using two-body parameters of Grimme-D3. If dftd3_version is set to
2
, three-body contribution is always disabled.
xdm_a1
- Type:
Float
- Default value:
0.6836
- GUI name:
a1
- Description:
Damping function parameter a1 (adimensional). It is NOT necessary to give a value if the functional is one of B86bPBE, PW86PBE, PBE, BLYP. For functionals in this list, the coefficients are given in: http://schooner.chem.dal.ca/wiki/XDM; A. Otero de la Roza, E. R. Johnson, J. Chem. Phys. 138, 204109 (2013) [doi:10.1063/1.4705760]
xdm_a2
- Type:
Float
- Default value:
1.5045
- Unit:
Angstrom
- GUI name:
a2
- Description:
Damping function parameter a2 (Angstrom). It is NOT necessary to give a value if the functional is one of B86bPBE, PW86PBE, PBE, BLYP. For functionals in this list, the coefficients are given in: http://schooner.chem.dal.ca/wiki/XDM; A. Otero de la Roza, E. R. Johnson, J. Chem. Phys. 138, 204109 (2013) [doi:10.1063/1.4705760]
Example values for xdm_a1 and xdm_a2 (source: postsg/xdm.param)
# quantum espresso, new version
functional a1 a2(ang) MAPD nset
b86bpbe (PAW) 0.6512 1.4633 11.8 49
pw86pbe (PAW) 0.6836 1.5045 11.7 49
blyp (PAW) 0.4502 1.6210 14.8 49
pbe (PAW) 0.3275 2.7673 14.4 49
b86bpbe (NC) 0.7767 1.0937 12.4 49
pw86pbe (NC) 0.7825 1.2077 12.6 49
blyp (NC) 0.6349 1.0486 11.2 49
pbe (NC) 0.4283 2.4690 15.2 49
# quantum espresso, new version, hybrids
functional a1 a2(ang) MAPD nset
hse (PAW) 0.3799 2.5862 10.5 49
pbe0 (PAW) 0.4616 2.2913 7.9 49
b3lyp (PAW) 0.6092 1.3452 8.5 49
b86bpbe 10% (PAW) 0.6470 1.4911 10.1 49
b86bpbe 20% (PAW) 0.6303 1.5579 8.8 49
b86bpbe 30% (PAW) 0.6134 1.6290 7.8 49
b86bpbe 40% (PAW) 0.5976 1.7000 7.1 49
b86bpbe 50% (PAW) 0.5826 1.7718 6.9 49
blyp 10% (PAW) 0.5637 1.4443 10.0 49
blyp 20% (PAW) 0.5663 1.5258 8.8 49
blyp 30% (PAW) 0.5174 1.7808 8.5 49
blyp 40% (PAW) 0.4195 2.1999 8.6 49
bhahlyp (PAW) 0.2998 2.6953 9.3 49
b3lyp (NC) 0.6070 1.3862 7.4 49
pbe0 (NC) 0.4590 2.3581 11.1 49
hse (NC) 0.4206 2.4989 11.9 49
b86bpbe 10% (NC) 0.7272 1.2674 10.8 49
b86bpbe 20% (NC) 0.6898 1.4072 9.6 49
b86bpbe 25% (NC) 0.6754 1.4651 9.2 49
b86bpbe 30% (NC) 0.6627 1.5181 9.0 49
b86bpbe 40% (NC) 0.6465 1.5981 8.9 49
b86bpbe 50% (NC) 0.6434 1.6405 9.1 49
blyp 10% (NC) 0.5967 1.3653 8.6 49
blyp 20% (NC) 0.5315 1.6669 7.8 49
blyp 30% (NC) 0.4398 2.0623 8.1 49
blyp 40% (NC) 0.3375 2.5011 9.1 49
bhahlyp (NC) 0.2292 2.9698 10.4 49
DFT functional (input_dft)¶
See also
System
input_dft string
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
input_dft
- Type:
String
- GUI name:
Density functional
- Description:
Exchange-correlation functional. Some valid values are • pbe • blyp • pbe0 • hse • revpbe • vdw-df-cx. See the documentation for more possible values. Overrides the value read from pseudopotential files.
Valid values for input_dft (source: Modules/funct.f90)
! ------------------------------------------------------------------------
! "dft" is the exchange-correlation functional label, as set by the user,
! using either set_dft_from_name or set_dft_from_indices. It can contain
! either the short names or a series of the keywords listed below.
! All operations on names are case-insensitive.
!
! short name complete name Short description
! "pz" = "sla+pz" = Perdew-Zunger LDA
! "bp" = "b88+p86" = Becke-Perdew grad.corr.
! "pw91" = "sla+pw+ggx+ggc" = PW91 (aka GGA)
! "blyp" = "sla+b88+lyp+blyp" = BLYP
! "pbe" = "sla+pw+pbx+pbc" = PBE
! "revpbe"= "sla+pw+revx+pbc" = revPBE (Zhang-Yang)
! "rpbe" = "sla+pw+hhnx+pbc" = RPBE (Hammer-Hansen-Norskov)
! "pw86pbe" = "sla+pw+pw86+pbc" = PW86 exchange + PBE correlation
! "b86bpbe" = "sla+pw+b86b+pbc" = B86b exchange + PBE correlation
! "pbesol"= "sla+pw+psx+psc" = PBEsol
! "q2d" = "sla+pw+q2dx+q2dc" = PBEQ2D
! "hcth" = "nox+noc+hcth+hcth" = HCTH/120
! "olyp" = "nox+lyp+optx+blyp" = OLYP
! "wc" = "sla+pw+wcx+pbc" = Wu-Cohen
! "sogga" = "sla+pw+sox+pbec" = SOGGA
! "optbk88"="sla+pw+obk8+p86" = optB88
! "optb86b"="sla+pw+ob86+p86" = optB86
! "ev93" = "sla+pw+evx+nogc" = Engel-Vosko
! "tpss" = "sla+pw+tpss+tpss" = TPSS Meta-GGA
! "m06l" = "nox+noc+m6lx+m6lc" = M06L Meta-GGA
! "tb09" = "sla+pw+tb09+tb09" = TB09 Meta-GGA
! "pbe0" = "pb0x+pw+pb0x+pbc" = PBE0
! "b86bx" = "pb0x+pw+b86x+pbc" = B86bPBE hybrid
! "bhahlyp"="pb0x+pw+b88x+blyp" = Becke half-and-half LYP
! "hse" = "sla+pw+hse+pbc" = Heyd-Scuseria-Ernzerhof (HSE 06, see note below)
! "b3lyp" = B3LYP
! "b3lyp-v1r" = B3LYP-VWN1-RPA
! "x3lyp" = X3LYP
! "vwn-rpa" = VWN LDA using vwn1-rpa parametrization
! "gaupbe"= "sla+pw+gaup+pbc" = Gau-PBE (also "gaup")
!
! "vdw-df" ="sla+pw+revx+vdw1" = vdW-DF1
! "vdw-df2" ="sla+pw+rw86+vdw2" = vdW-DF2
! "vdw-df-c09" ="sla+pw+c09x+vdw1" = vdW-DF-C09
! "vdw-df2-c09" ="sla+pw+c09x+vdw2" = vdW-DF2-C09
! "vdw-df-obk8" ="sla+pw+obk8+vdw1" = vdW-DF-obk8 (optB88-vdW)
! "vdw-df-ob86" ="sla+pw+ob86+vdw1" = vdW-DF-ob86 (optB86b-vdW)
! "vdw-df2-b86r" ="sla+pw+b86r+vdw2" = vdW-DF2-B86R (rev-vdw-df2)
! "vdw-df-cx" ="sla+pw+cx13+vdW1" = vdW-DF-cx
! "vdw-df-cx0" ="sla+pw+cx13+vdW1+HF/4" = vdW-DF-cx-0
! "vdw-df2-0" ="sla+pw+rw86+vdw2+HF/4" = vdW-DF2-0
! "vdw-df2-br0" ="sla+pw+b86r+vdW2+HF/4" = vdW-DF2-b86r-0
! "vdw-df-c090" ="sla+pw+c09x+vdw1+HF/4" = vdW-DF-C09-0
! "vdw-df3-opt1" ="sla+pw+w31x+w31c" = vdW-DF3-opt1
! "vdw-df3-opt2" ="sla+pw+w32x+w32c" = vdW-DF3-opt2
! "vdw-df-C6" ="sla+pw+b86r+wc6" = vdW-DF-C6
! "rvv10" = "sla+pw+rw86+pbc+vv10" = rVV10
!
! Any nonconflicting combination of the following keywords is acceptable:
!
! Exchange: "nox" none iexch=0
! "sla" Slater (alpha=2/3) iexch=1 (default)
! "sl1" Slater (alpha=1.0) iexch=2
! "rxc" Relativistic Slater iexch=3
! "oep" Optimized Effective Potential iexch=4
! "hf" Hartree-Fock iexch=5
! "pb0x" (Slater*0.75+HF*0.25) iexch=6 for PBE0 and vdW-DF-cx0 and vdW-DF2-0 etc
! "b3lp" B3LYP(Slater*0.80+HF*0.20) iexch=7
! "kzk" Finite-size corrections iexch=8
! "x3lp" X3LYP(Slater*0.782+HF*0.218) iexch=9
! "kli" KLI aproximation for exx iexch=10
!
! Correlation: "noc" none icorr=0
! "pz" Perdew-Zunger icorr=1 (default)
! "vwn" Vosko-Wilk-Nusair icorr=2
! "lyp" Lee-Yang-Parr icorr=3
! "pw" Perdew-Wang icorr=4
! "wig" Wigner icorr=5
! "hl" Hedin-Lunqvist icorr=6
! "obz" Ortiz-Ballone form for PZ icorr=7
! "obw" Ortiz-Ballone form for PW icorr=8
! "gl" Gunnarson-Lunqvist icorr=9
! "kzk" Finite-size corrections icorr=10
! "vwn-rpa" Vosko-Wilk-Nusair, alt param icorr=11
! "b3lp" B3LYP (0.19*vwn+0.81*lyp) icorr=12
! "b3lpv1r" B3LYP-VWN-1-RPA
! (0.19*vwn_rpa+0.81*lyp) icorr=13
! "x3lp" X3LYP (0.129*vwn_rpa+0.871*lyp)icorr=14
!
! Gradient Correction on Exchange:
! "nogx" none igcx =0 (default)
! "b88" Becke88 (beta=0.0042) igcx =1
! "ggx" Perdew-Wang 91 igcx =2
! "pbx" Perdew-Burke-Ernzenhof exch igcx =3
! "revx" revised PBE by Zhang-Yang igcx =4
! "hcth" Cambridge exch, Handy et al igcx =5
! "optx" Handy's exchange functional igcx =6
! "pb0x" PBE0 (PBE exchange*0.75) igcx =8
! "b3lp" B3LYP (Becke88*0.72) igcx =9
! "psx" PBEsol exchange igcx =10
! "wcx" Wu-Cohen igcx =11
! "hse" HSE screened exchange igcx =12
! "rw86" revised PW86 igcx =13
! "pbe" same as PBX, back-comp. igcx =14
! "c09x" Cooper 09 igcx =16
! "sox" sogga igcx =17
! "q2dx" Q2D exchange grad corr igcx =19
! "gaup" Gau-PBE hybrid exchange igcx =20
! "pw86" Perdew-Wang (1986) exchange igcx =21
! "b86b" Becke (1986) exchange igcx =22
! "obk8" optB88 exchange igcx =23
! "ob86" optB86b exchange igcx =24
! "evx" Engel-Vosko exchange igcx =25
! "b86r" revised Becke (b86b) igcx =26
! "cx13" consistent exchange igcx =27
! "x3lp" X3LYP (Becke88*0.542 +
! Perdew-Wang91*0.167) igcx =28
! "cx0" vdW-DF-cx+HF/4 (cx13-0) igcx =29
! "r860" rPW86+HF/4 (rw86-0) igcx =30 (for DF0)
! "cx0p" vdW-DF-cx+HF/5 (cx13-0p) igcx =31
! "ahcx" vdW-DF-cx based analytic hole igcx =32 ! Launched vdW-DF-ahcx - PH
! "ahf2" vdW-DF2 based analytic hole igcx =33 ! Defined vdw-DF2-AH at 0.20 - PH
! "ahpb" PBE based analytic hole igcx =34 ! PBE-AH (rHJS-PBE) at 0.20 - PH
! "ahps" PBE-sol based analytic hole igcx =35 ! PBESOL-AH (rHJS-PBEsol) at 0.20 - PH
! "cx14" Exporations igcx =36 reserved PH
! "cx15" Exporations igcx =37 reserved PH
! "br0" vdW-DF2-b86r+HF/4 (b86r-0) igcx =38
! "cx16" Exporations igcx =39 reserved PH
! "c090" vdW-DF-c09+HF/4 (c09-0) igcx =40
! "b86x" B86b exchange * 0.75 igcx =41
! "b88x" B88 exchange * 0.50 igcx =42
! "beex" BEE exchange igcx =43
! "hhnx" Hammer-Hansen-Norskov igcx =44
! "w31x" vdW-DF3-opt1 exchange igcx =45
! "w32x" vdW-DF3-opt2 exchange igcx =46
! "ahtr" vdW-DF2-ahtr exchange igcx =47 ! Test reserve called by vdW-DF2-ahtr - PH
! "ehpb" HSE variant igcx =48 ! Reserved PH
! "hjpb" HJS-type PBE cross check igcx =49 ! Reserved PH
! "hjps" HJS-type PBEsol crosscheck igcx =50 ! Reserved PH
!
! Gradient Correction on Correlation:
! "nogc" none igcc =0 (default)
! "p86" Perdew86 igcc =1
! "ggc" Perdew-Wang 91 corr. igcc =2
! "blyp" Lee-Yang-Parr igcc =3
! "pbc" Perdew-Burke-Ernzenhof corr igcc =4
! "hcth" Cambridge corr, Handy et al igcc =5
! "b3lp" B3LYP (Lee-Yang-Parr*0.81) igcc =7
! "psc" PBEsol corr igcc =8
! "pbe" same as PBX, back-comp. igcc =9
! "q2dc" Q2D correlation grad corr igcc =12
! "x3lp" X3LYP (Lee-Yang-Parr*0.871) igcc =13
! "beec" BEE correlation igcc =14
!
! Meta-GGA functionals
! "tpss" TPSS Meta-GGA imeta=1
! "m6lx" M06L Meta-GGA imeta=2
! "tb09" TB09 Meta-GGA imeta=3
! "+meta" activate MGGA even without MGGA-XC imeta=4
! "scan" SCAN Meta-GGA imeta=5
! "sca0" SCAN0 Meta-GGA imeta=6
! "r2scan" R2SCAN Meta-GGA imeta=7
!
! van der Waals functionals (nonlocal term only)
! "nonlc" none inlc =0 (default)
!--------------inlc = 1 to inlc = 25 reserved for vdW-DF--------------
! "vdw1" vdW-DF1 inlc =1
! "vdw2" vdW-DF2 inlc =2
! "w31c" vdW-DF3-opt1 inlc =3
! "w32c" vdW-DF3-opt2 inlc =4
! "wc6" vdW-DF-C6 inlc =5
!---------------------------------------------------------------------
! "vv10" rVV10 inlc =26
!
! Meta-GGA with van der Waals
! "rvv10-scan" rVV10 (with b=15.7) and scan inlc=26 (PRX 6, 041005 (2016))
!
! Note: as a rule, all keywords should be unique, and should be different
! from the short name, but there are a few exceptions.
!
! References:
! pz J.P.Perdew and A.Zunger, PRB 23, 5048 (1981)
! vwn S.H.Vosko, L.Wilk, M.Nusair, Can.J.Phys. 58,1200(1980)
! vwn1-rpa S.H.Vosko, L.Wilk, M.Nusair, Can.J.Phys. 58,1200(1980)
! wig E.P.Wigner, Trans. Faraday Soc. 34, 67 (1938)
! hl L.Hedin and B.I.Lundqvist, J. Phys. C4, 2064 (1971)
! gl O.Gunnarsson and B.I.Lundqvist, PRB 13, 4274 (1976)
! pw J.P.Perdew and Y.Wang, PRB 45, 13244 (1992)
! obpz G.Ortiz and P.Ballone, PRB 50, 1391 (1994)
! obpw as above
! b88 A.D.Becke, PRA 38, 3098 (1988)
! p86 J.P.Perdew, PRB 33, 8822 (1986)
! pw86 J.P.Perdew, PRB 33, 8800 (1986)
! b86b A.D.Becke, J.Chem.Phys. 85, 7184 (1986)
! ob86 Klimes, Bowler, Michaelides, PRB 83, 195131 (2011)
! b86r I. Hamada, Phys. Rev. B 89, 121103(R) (2014)
! w31x D. Chakraborty, K. Berland, and T. Thonhauser, JCTC 16, 5893 (2020)
! w32x D. Chakraborty, K. Berland, and T. Thonhauser, JCTC 16, 5893 (2020)
! pbe J.P.Perdew, K.Burke, M.Ernzerhof, PRL 77, 3865 (1996)
! pw91 J.P.Perdew and Y. Wang, PRB 46, 6671 (1992)
! blyp C.Lee, W.Yang, R.G.Parr, PRB 37, 785 (1988)
! hcth Handy et al, JCP 109, 6264 (1998)
! olyp Handy et al, JCP 116, 5411 (2002)
! revPBE Zhang and Yang, PRL 80, 890 (1998)
! pbesol J.P. Perdew et al., PRL 100, 136406 (2008)
! q2d L. Chiodo et al., PRL 108, 126402 (2012)
! rw86 Eamonn D. Murray et al, J. Chem. Theory Comput. 5, 2754 (2009)
! wc Z. Wu and R. E. Cohen, PRB 73, 235116 (2006)
! kzk H.Kwee, S. Zhang, H. Krakauer, PRL 100, 126404 (2008)
! pbe0 J.P.Perdew, M. Ernzerhof, K.Burke, JCP 105, 9982 (1996)
! hse Heyd, Scuseria, Ernzerhof, J. Chem. Phys. 118, 8207 (2003)
! Heyd, Scuseria, Ernzerhof, J. Chem. Phys. 124, 219906 (2006).
! b3lyp P.J. Stephens,F.J. Devlin,C.F. Chabalowski,M.J. Frisch
! J.Phys.Chem 98, 11623 (1994)
! x3lyp X. Xu, W.A Goddard III, PNAS 101, 2673 (2004)
! vdW-DF M. Dion et al., PRL 92, 246401 (2004)
! T. Thonhauser et al., PRL 115, 136402 (2015)
! vdW-DF2 Lee et al., Phys. Rev. B 82, 081101 (2010)
! rev-vdW-DF2 I. Hamada, Phys. Rev. B 89, 121103(R) (2014)
! vdW-DF-cx K. Berland and P. Hyldgaard, PRB 89, 035412 (2014)
! vdW-DF-cx0 K. Berland, Y. Jiao, J.-H. Lee, T. Rangel, J. B. Neaton and P. Hyldgaard,
! J. Chem. Phys. 146, 234106 (2017)
! vdW-DF-cx0p Y. Jiao, E. Schröder and P. Hyldgaard,
! J. Chem. Phys. 148, 194115 (2018)
! vdW-DF-obk8 Klimes et al, J. Phys. Cond. Matter, 22, 022201 (2010)
! vdW-DF-ob86 Klimes et al, Phys. Rev. B, 83, 195131 (2011)
! vdW-DF3-opt1 D. Chakraborty, K. Berland, and T. Thonhauser, JCTC 16, 5893 (2020)
! vdW-DF3-opt2 D. Chakraborty, K. Berland, and T. Thonhauser, JCTC 16, 5893 (2020)
! vdW-DF-C6 K. Berland, D. Chakraborty, and T. Thonhauser, PRB 99, 195418 (2019)
! c09x V. R. Cooper, Phys. Rev. B 81, 161104(R) (2010)
! tpss J.Tao, J.P.Perdew, V.N.Staroverov, G.E. Scuseria,
! PRL 91, 146401 (2003)
! tb09 F Tran and P Blaha, Phys.Rev.Lett. 102, 226401 (2009)
! scan J Sun, A Ruzsinszky and J Perdew, PRL 115, 36402 (2015)
! scan0 K Hui and J-D. Chai, JCP 144, 44114 (2016)
! r2scan J. W. Furness, A. D. Kaplan, J. Ning, J. P. Perdew,
! and J. Sun, JPCL 11, 8208 (2020)
! sogga Y. Zhao and D. G. Truhlar, JCP 128, 184109 (2008)
! m06l Y. Zhao and D. G. Truhlar, JCP 125, 194101 (2006)
! gau-pbe J.-W. Song, K. Yamashita, K. Hirao JCP 135, 071103 (2011)
! rVV10 R. Sabatini et al. Phys. Rev. B 87, 041108(R) (2013)
! ev93 Engel-Vosko, Phys. Rev. B 47, 13164 (1993)
! vdW-DF-ahcx V. Shukla, Y. Jiao, iC. M. Frostenson, and P. Hyldgaard, JPCM 34, 025902 (2022)
! vdW-DF2-ah V. Shukla, Y. Jiao, iC. M. Frostenson, and P. Hyldgaard, JPCM 34, 025902 (2022)
! PBE-ah V. Shukla, Y. Jiao, iC. M. Frostenson, and P. Hyldgaard, JPCM 34, 025902 (2022)
! PBESOL-ah V. Shukla, Y. Jiao, iC. M. Frostenson, and P. Hyldgaard, JPCM 34, 025902 (2022)
!
! NOTE ABOUT HSE: there are two slight deviations with respect to the HSE06
! functional as it is in Gaussian code (that is considered as the reference
! in the chemistry community):
! - The range separation in Gaussian is precisely 0.11 bohr^-1,
! instead of 0.106 bohr^-1 in this implementation
! - The gradient scaling relation is a bit more complicated
! [ see: TM Henderson, AF Izmaylov, G Scalmani, and GE Scuseria,
! J. Chem. Phys. 131, 044108 (2009) ]
! These two modifications accounts only for a 1e-5 Ha difference for a
! single He atom. Info by Fabien Bruneval.
!
! NOTE FOR LIBXC USERS: to use libxc functionals you must enforce them from input (use
! 'input_dft' in &system) and write their IDs in the input string. The only notation
! now allowed (v7.0) for input DFTs containing Libxc terms is:
! XC-000i-000i-000i-000i-000i-000i
! where you put the functional IDs instead of the zeros and an 'L' instead of
! 'i' if the functional is from Libxc. The order is the usual one:
! LDAexch - LDAcorr - GGAexch - GGAcorr - MGGAexch - MGGAcorr
! however QE will automatically adjust it if needed. You can skip zero tails (e.g.
! you don't need GGA/MGGA slots if the dft is LDA only and so on.
! You can use combinations of qe and libxc functionals, when they are compatible.
! You can also add vdW terms after it, for example, sla+pw+rw86+vdw2 is:
! input_dft='XC-001i-004i-013i-vdw2'.
! For more details see the user_guide (in 'Doc' folder).
Exact exchange (EXX)¶
See also
System
ecutfock float
ecutvcut float
exxdiv_treatment [gygi-baldereschi | vcut_spherical | vcut_ws | none]
exx_fraction float
nqx1 integer
nqx2 integer
nqx3 integer
screening_parameter float
x_gamma_extrapolation Yes/No
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
ecutfock
- Type:
Float
- Unit:
Rydberg
- GUI name:
Exchange operator cutoff
- Description:
Kinetic energy cutoff for the exact exchange operator in EXX type calculations. By default this is the same as
ecutrho
but in some EXX calculations, a significant speed-up can be obtained by reducing ecutfock, at the expense of some loss in accuracy. Must be >=ecutwfc
. Not implemented for stress calculation and for US-PP and PAW pseudopotentials. Use with care, especially in metals where it may give raise to instabilities.
ecutvcut
- Type:
Float
- Default value:
0.0
- Unit:
Rydberg
- Description:
Reciprocal space cutoff for correcting Coulomb potential divergencies at small q vectors.
exxdiv_treatment
- Type:
Multiple Choice
- Default value:
gygi-baldereschi
- Options:
[gygi-baldereschi, vcut_spherical, vcut_ws, none]
- GUI name:
Divergence treatment
- Description:
Specific for EXX. It selects the kind of approach to be used for treating the Coulomb potential divergencies at small q vectors. gygi-baldereschi: appropriate for cubic and quasi-cubic supercells vcut_spherical: appropriate for cubic and quasi-cubic supercells vcut_ws: appropriate for strongly anisotropic supercells, see also ecutvcut. none: sets Coulomb potential at G,q=0 to 0.0 (required for GAU-PBE)
exx_fraction
- Type:
Float
- GUI name:
EXX fraction
- Description:
Fraction of EXX for hybrid functional calculations. In the case of
input_dft
set to ‘PBE0’, the default value is 0.25, while forinput_dft
set to ‘B3LYP’ theexx_fraction
default value is 0.20.
nqx1
- Type:
Integer
- Description:
Three-dimensional mesh for q (k1-k2) sampling of the Fock operator (EXX). Can be smaller than the number of k-points. Defaults to the size of the k-point mesh used.
nqx2
- Type:
Integer
- Description:
Three-dimensional mesh for q (k1-k2) sampling of the Fock operator (EXX). Can be smaller than the number of k-points. Defaults to the size of the k-point mesh used.
nqx3
- Type:
Integer
- Description:
Three-dimensional mesh for q (k1-k2) sampling of the Fock operator (EXX). Can be smaller than the number of k-points. Defaults to the size of the k-point mesh used.
screening_parameter
- Type:
Float
- Default value:
0.106
- GUI name:
Screening parameter
- Description:
screening_parameter for HSE like hybrid functionals. For more information, see: J. Chem. Phys. 118, 8207 (2003), doi:10.1063/1.1564060 J. Chem. Phys. 124, 219906 (2006), doi:10.1063/1.2204597
x_gamma_extrapolation
- Type:
Bool
- Default value:
Yes
- GUI name:
Gamma extrapolation
- Description:
Specific for EXX. If .true., extrapolate the G=0 term of the potential (see README in examples/EXX_example for more) Set this to .false. for GAU-PBE.
Dipole/charge corrections¶
See also
System
edir [1 | 2 | 3]
emaxpos float
eopreg float
eamp float
assume_isolated [Auto | None | Martyna-Tuckerman | ESM | 2D]
End
System
- Type:
Block
- Description:
Keywords from the &SYSTEM namelist in the QuantumEspresso input file.
edir
- Type:
Multiple Choice
- Options:
[1, 2, 3]
- GUI name:
Field direction
- Description:
The direction of the electric field or dipole correction is parallel to the bg(:,edir) reciprocal lattice vector. Thus the potential is constant in planes defined by FFT grid points. Used only if
tefield
is enabled.
emaxpos
- Type:
Float
- Default value:
0.5
- GUI name:
Saw potential maximum
- Description:
Position of the maximum of the saw-like potential along crystal axis
edir
, within the unit cell, see alsoeopreg
. 0 <emaxpos
< 1 Used only iftefield
is enabled.
eopreg
- Type:
Float
- Default value:
0.1
- GUI name:
Saw potential decreasing
- Description:
Zone in the unit cell where the saw-like potential decreases, see also
amp
. Must be in range 0 <eopreg
< 1. Used only iftefield
is enabled.
eamp
- Type:
Float
- Default value:
0.001
- Unit:
Hartree
- GUI name:
Field amplitude
- Description:
Amplitude of the electric field, in Hartree a.u. = = 51.4220632*10^10 V/m. Used only if
tefield
is enabled. The saw-like potential increases with slopeeamp
in the region from (emaxpos
+eopreg
- 1) to (emaxpos
), then decreases to 0 until (emaxpos
+eopreg
), in units of the crystal vector edir. Important: the change of slope of this potential must be located in the empty region, or else unphysical forces will result.
assume_isolated
- Type:
Multiple Choice
- Default value:
Auto
- Options:
[Auto, None, Martyna-Tuckerman, ESM, 2D]
- GUI name:
Isolated system
- Description:
Used to perform calculation assuming the system to be isolated (a molecule or a cluster in a 3D supercell). Currently available choices: • Auto: determines the used method based on the periodicity of the system in the AMS driver input. None for systems 3D periodicity, Martyna-Tuckerman for systems without a lattice. • None: regular periodic calculation w/o any correction. • Martyna-Tuckerman: correction to both total energy and scf potential. Adapted from: G.J. Martyna, and M.E. Tuckerman, A reciprocal space based method for treating long range interactions in ab-initio and force-field-based calculation in clusters, J. Chem. Phys. 110, 2810 (1999), [doi:10.1063/1.477923]. • ESM: Effective Screening Medium Method. For polarized or charged slab calculation, embeds the simulation cell within an effective semi-infinite medium in the perpendicular direction (along z). Embedding regions can be vacuum or semi-infinite metal electrodes (use esm_bc to choose boundary conditions). If between two electrodes, an optional electric field (esm_efield) may be applied. Method described in M. Otani and O. Sugino, ‘First-principles calculations of charged surfaces and interfaces: A plane-wave nonrepeated slab approach’, PRB 73, 115407 (2006). • 2D: Truncation of the Coulomb interaction in the z direction for structures periodic in the x-y plane. Total energy, forces and stresses are computed in a two-dimensional framework. Linear-response calculations () done on top of a self-consistent calculation with this flag will automatically be performed in the 2D framework as well. Please refer to: Sohier, T., Calandra, M., & Mauri, F. (2017), ‘Density functional perturbation theory for gated two-dimensional heterostructures: Theoretical developments and application to flexural phonons in graphene’, PRB, 96, 075448 (2017).
Hubbard U, DFT+U¶
Note: the Hubbard U (and J) settings are specified in the Quantum ESPRESSO 7.1 format (pdf)
.
This format is different compared to earlier versions of Quantum ESPRESSO. See the Examples for example usage in AMS.
Example: DFT+U (Dudarev’s formalism)¶
Hubbard ortho-atomic
U Mn-3d 5.0 # eV
U Ni-3d 6.0 # eV
End
Instead of 3d
, you can also specify for example 4s
etc.
To apply the Hund J0 (DFT+U+J0):
Hubbard ortho-atomic
U Mn-3d 5.0 # eV
J0 Mn-3d 1.0 # eV
U Ni-3d 6.0 # eV
J0 Ni-3d 1.2 # eV
End
Example: DFT+U+J (Liechtenstein’s formulation)¶
Hubbard ortho-atomic
U Mn-3d 5.0
J Mn-3d 1.0
B Mn-3d 1.1
End
For details, see the Quantum ESPRESSO documentation for Hubbard U (pdf)
.
Hubbard
- Type:
Non-standard block
- Description:
Specify parameters for DFT+U models. The type of Hubbard projectors to use (e.g.
atomic
orortho-atomic
is specified in the header of this block. Example input: Hubbard ortho-atomic U Fe-3d 3.0 End More examples can be found in the documentation.
Properties:¶
Properties
BandStructure Yes/No
DOS Yes/No
NormalModes Yes/No
Phonons Yes/No
WorkFunction Yes/No
End
Properties
- Type:
Block
- Description:
Configures which QE level properties to calculate for SinglePoint calculations or other important geometries (e.g. at the end of an optimization).
BandStructure
- Type:
Bool
- Default value:
No
- GUI name:
Calculate band structure
- Description:
If true, the band structure is calculated and saved for visualization. To configure the parameters of the calculation, please modify the options in the the section ‘BandStructure’.
DOS
- Type:
Bool
- Default value:
No
- GUI name:
Calculate DOS
- Description:
If true, the Density-Of-States (DOS) is calculated and saved for visualization. To configure the parameters of the calculation, please modify the options in the the section ‘DOS’.
NormalModes
- Type:
Bool
- Default value:
No
- GUI name:
Frequencies
- Description:
If true, frequencies and normal modes of vibration are calculated and saved for visualization. To configure the parameters of the calculation, please modify the options in the the section ‘NormalModes’.
Phonons
- Type:
Bool
- Default value:
No
- GUI name:
Calculate Phonons
- Description:
If true, the phonons are calculated and saved for visualization. To configure the parameters of the calculation, please modify the options in the the section ‘Phonons’.
WorkFunction
- Type:
Bool
- Default value:
No
- GUI name:
Calculate work function
- Description:
If true, the work function is calculated and saved for visualization. To configure the parameters of the calculation, please modify the options in the the section ‘WorkFunction’.
Density of states: DOS, PDOS¶
DOS
DeltaE float
Emax float
Emin float
K_Points header # Non-standard block. See details.
...
End
K_PointsStep float
PDOS Yes/No
degauss float
nbnd integer
ngauss [SimpleGaussian | Methfessel-Paxton | ColdSmearing | Fermi-Dirac | Default]
occupations [Smearing | Tetrahedra | Tetrahedra_lin | Tetrahedra_opt | Fixed | Auto]
End
DOS
- Type:
Block
- Description:
This section configures the parameters for calculating the Density of States (DOS). These are the utilities involved: •
kpath
: This AMS tool generates an automated high-symmetry k-path in the Brillouin zone. •pw.x
(withcalculation=nscf
): This Quantum ESPRESSO (QE) utility conducts electronic structure calculations, specifically for the non-self-consistent field (nscf) computation. •dos.x
: A QE utility utilized for post-processing electronic structure calculations. It analyzes the electronic wavefunctions obtained from preceding calculations to determine the density of available electronic states at different energy levels. For more details see https://www.quantum-espresso.org/Doc/INPUT_DOS.html •projwfc.x
: Another QE utility employed for post-processing electronic structure calculations. It projects the wavefunctions onto atomic orbitals or basis sets, offering insights into the composition and character of electronic states. For more details see https://www.quantum-espresso.org/Doc/INPUT_PROJWFC.html By default, the calculation sequence follows the order:kpath -> pw.x(calculation=nscf) -> dos.x
. However, enablingDOS%PDOS
switches the calculation to useprojwfc.x
instead ofdos.x
. While common parameters can be customized directly in this section, specialized adjustments should be made in either theDOS_X
orPROJWFC_X
section, depending on specific requirements.
DeltaE
- Type:
Float
- Default value:
0.1
- Unit:
eV
- GUI name:
Energy step
- Description:
Energy grid step.
Emax
- Type:
Float
- Unit:
eV
- Description:
Maximum energy for DOS plot. If unspecified, the upper band value, plus 3 times the value of the gaussian smearing if present, will be used.
Emin
- Type:
Float
- Unit:
eV
- Description:
Minimum energy for DOS plot. If unspecified, the lower band value, minus 3 times the value of the gaussian smearing if present, will be used.
K_Points
- Type:
Non-standard block
- Description:
Specify the k-points to use. Choose a header appropriate for your system. Available values are:
tpiba
,automatic
,crystal
,gamma
,tpiba_b
,crystal_b
,tpiba_c
,crystal_c
, andams_kpath
. See the QE documentation for details. If omitted, the k-points specified in the main QE calculation will be used. For most cases,automatic
(which generates a Monkhorst-Pack grid) is recommended.
K_PointsStep
- Type:
Float
- Default value:
0.05
- Unit:
1/Bohr
- Description:
This option is used only if the header of the
DOS%K_Points
block isams_kpath
.
PDOS
- Type:
Bool
- Default value:
No
- GUI name:
Calculate PDOS and Lowdin charges
- Description:
If true, the partial Density-Of-States (projections on atomic basis functions) is calculated and saved for visualization. It uses the QE-utility
projwfc.x
. To configure the parameters of the calculation, please modify the options in the the sectionPROJWFC_X
.
degauss
- Type:
Float
- Unit:
Rydberg
- GUI name:
Broadening width
- Description:
Gaussian broadening. See more details in sections
DOS_X
orPROJWFC_X
.
nbnd
- Type:
Integer
- GUI name:
Number of bands
- Description:
Number of electronic states (bands) to be calculated. Note that in spin-polarized calculations the number of k-point, not the number of bands per k-point, is doubled. Default: 20% more (minimum of 4 additional bands) than the number used in the main ‘pw.x’ calculation, regardless of the material’s insulating or metallic nature. Notice that this default is calculated differently than in standard QE.
ngauss
- Type:
Multiple Choice
- Default value:
Default
- Options:
[SimpleGaussian, Methfessel-Paxton, ColdSmearing, Fermi-Dirac, Default]
- GUI name:
Broadening type
- Description:
Type of gaussian broadening: Available options are: • SimpleGaussian. • Methfessel-Paxton: Methfessel-Paxton of order 1. • ColdSmearing: Marzari-Vanderbilt-DeVita-Payne. • Fermi-Dirac: Fermi-Dirac function. • Default: See more details in sections
DOS_X
orPROJWFC_X
.
occupations
- Type:
Multiple Choice
- Default value:
Auto
- Options:
[Smearing, Tetrahedra, Tetrahedra_lin, Tetrahedra_opt, Fixed, Auto]
- GUI name:
Non-SCF Occupations
- Description:
Available options are: • Smearing: gaussian smearing for metals; see keywords
smearing
anddegauss
• Tetrahedra: Tetrahedron method, Bloechl’s version: P.E. Bloechl, PRB 49, 16223 (1994). Requires uniform grid of k-points, to be automatically generated (seeblock K_Points
). Well suited for calculation of DOS, less so (because not variational) for force/optimization/dynamics calculations. • Tetrahedra_lin: Original linear tetrahedron method. To be used only as a reference; the optimized tetrahedron method is more efficient. • Tetrahedra_opt: optimized tetrahedron method, see M. Kawamura, PRB 89, 094515 (2014). Can be used for phonon calculations as well. • Fixed: for insulators with a gap. • Auto: UsesTetrahedra
for 3D and 2D systems, andFixed
for 0D and 1D systems.
Electronic band structure¶
Before calculating the band structure, make sure that the crystal unit cell corresponds to the primitive unit cell!
BandStructure
K_Points header # Non-standard block. See details.
...
End
K_PointsLabels string
K_PointsStep float
nbnd integer
End
BandStructure
- Type:
Block
- Description:
This section configures the parameters for calculating the Band Structure. This involves utilizing the following utilities in sequential order: •
kpath
: This AMS tool generates an automated high-symmetry k-path in the Brillouin zone. •pw.x
(with calculation=bands): This utility from Quantum ESPRESSO (QE) performs electronic structure calculations, particularly for bands. For more details see https://www.quantum-espresso.org/Doc/INPUT_PW.html •bands.x
: Another QE utility, which calculates the band structure. For more details see https://www.quantum-espresso.org/Doc/INPUT_BANDS.html.
K_Points
- Type:
Non-standard block
- Description:
Specify the k-points to use. Choose a header appropriate for your system. Available values are:
tpiba
,automatic
,crystal
,gamma
,tpiba_b
,crystal_b
,tpiba_c
,crystal_c
, andams_kpath
. See the QE documentation for details. If omitted,ams_kpath
will be used for 3D systems, andgamma
otherwise. For most cases,ams_kpath
(which generates a convenient path along high-symmetry k-points in the Brillouin zone) is recommended.
K_PointsLabels
- Type:
String
- Description:
You can provide labels for your k-points, like L-G-X-U-G, separating each label with a hyphen (-) or a vertical bar (|). For example, L-G-X-U-G and L|G|X|U|G are both valid. These labels are optional and only used for display purposes when the
K_Points
block is specified. This option is used only if the header of theBandStructure%K_Points
block isams_kpath
. **Important:** These labels do not determine the actual k-point coordinates. You must specify the k-point coordinates separately within theK_Points
section.
K_PointsStep
- Type:
Float
- Default value:
0.05
- Unit:
1/Bohr
- Description:
This option is used only if the header of the
BandStructure%K_Points
block isams_kpath
.
nbnd
- Type:
Integer
- GUI name:
Number of bands
- Description:
Number of electronic states (bands) to be calculated. Note that in spin-polarized calculations the number of k-point, not the number of bands per k-point, is doubled. Default: 20% more (minimum of 4 additional bands) than the number used in the main ‘pw.x’ calculation, regardless of the material’s insulating or metallic nature. Notice that this default is calculated differently than in standard QE.
Work function¶
WorkFunction
centralize Yes/No
idir [1 | 2 | 3]
npt integer
End
WorkFunction
- Type:
Block
- Description:
This section configures the parameters for calculating the Work Function. This involves utilizing the following utilities in sequential order: •
pp.x
: Calculates the the electrostatic potential using the results from the last Quantum ESPRESSO calculation. •average.x
: Performs planar and macroscopic averages of the electrostatic potential along a specified direction, which are crucial for determining the vacuum level and subsequently the work function.
centralize
- Type:
Bool
- Default value:
Yes
- Description:
Translates the calculated electrostatic potential along the ‘idir’ coordinate, respecting periodic boundary conditions, so that the geometric center of the system is at the center of the coordinate.
idir
- Type:
Multiple Choice
- Default value:
3
- Options:
[1, 2, 3]
- Description:
1, 2 or 3. Planar average is done in the plane orthogonal to direction
idir
, as defined for the crystal cell. Theidir
parameter defaults to the value ofSystem%edir
if it’s set. Otherwise,idir
is set to 3.
npt
- Type:
Integer
- Description:
Number of points used for the final interpolation of the planar and macroscopic averages of the electrostatic potential. This controls the resolution of the averaged potential data. If npt is less than or equal to N_idir (the number of FFT grid points along the specified direction), no interpolation is performed and the raw FFT data is used. The default value is 10 * N_idir, which typically provides sufficient resolution for accurate work function calculations.
Expert input for post-processing¶
DOS_X (dos.x)¶
Warning
Use the DOS_X
input block only if you cannot achieve your goal using the DOS
block.
Input options for the dos.x program.
PROJWFC_X (projwfc.x)¶
Input options for the projwfc.x program.
Differences between AMS and standalone QE¶
AMS enforces
scf_must_converge = .false.
The default value for
Electrons%mixing_beta
is 0.3 (smaller than the pw.x default of 0.7), to make SCF convergence more reliable.The pseudopotentials are specified in the engine Pseudopotentials block. They will then be appended to the ATOMIC_SPECIES lines in the pw.x input.
AMS automatically sets
pseudo_dir
,outdir
,prefix
,title
,ntyp
andnat
AMS automatically generates a path through the Brillouin zone for band structure calculations by default
For more differences, see the Quick reference (migration guide)